Popular

Heliophysics Events Knowledgebase Coverage Registry (HCR)

Popular Observations

Here are the most popular observations, as measured by the number of downloads.

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247296 matches
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IRIS: Solar orbiter SPICE

2022-11-03T06:28:15 to 2022-11-03T07:41:44

Science Goal: Very large sparse 96-step raster 95x175 96s C II Si IV Mg II h/k Deep x 8 Spatial x 2, Spectral x 2 FUV spectrally rebinned x 4

Program: Solar orbiter SPICE

Target: QS

Pointing: xcen=-484 ycen=73,

saaIntervals hiIntervals

wavelength	cadence	FOVx,y	images
1330	0.46	264,182	160
1400	0.46	264,182	160
2796	0.46	264,182	160

IRIS: High Cadence Flare program

2022-11-03T00:13:22 to 2022-11-03T01:18:46

Science Goal: High-Cadence Flare Program: .3 sec, flare linelist, Mg II h/k slow

Program: High Cadence Flare program

Target: AR

Pointing: xcen=35 ycen=374,

saaIntervals hiIntervals

wavelength	cadence	FOVx,y	images
2796	0.16	61,68	399

IRIS: Solar orbiter SPICE

2022-10-30T01:46:14 to 2022-10-30T02:35:48

Science Goal: Very large dense 320-step raster 105.3x175 320s C II Si IV Mg II h/k Deep x 8 FUV spectrally rebinned x 4

Program: Solar orbiter SPICE

Target: QS

Pointing: xcen=-590 ycen=66,

saaIntervals hiIntervals

wavelength	cadence	FOVx,y	images
1330	0.62	281,182	80
1400	0.62	281,182	80
2796	0.62	281,182	80

IRIS: A1: QS monitoring

2022-10-29T01:10:37 to 2022-10-29T01:28:41

Science Goal: Large coarse 64-step raster 126x120 64s C II Si IV Mg II h/k Mg II w s Deep x 15 SJI cadence 0.5x faster

Program: A1: QS monitoring

Target: QS

Pointing: xcen=0 ycen=2,

saaIntervals hiIntervals

wavelength	cadence	FOVx,y	images
1330	1.13	247,129	16
2832	4.52	247,129	4
1400	1.13	247,129	16
2796	1.13	247,129	16

IRIS: Solar Orbiter: SPICE

2022-10-22T10:33:42 to 2022-10-22T14:19:24

Science Goal: Very large coarse 64-step raster 126x175 64s C II Si IV Mg II h/k Deep x 8 Spatial x 2, Spectral x 2

Program: Solar Orbiter: SPICE

Target: AR

Pointing: xcen=-774 ycen=219,

saaIntervals hiIntervals

wavelength	cadence	FOVx,y	images
1330	0.61	295,182	368
1400	0.61	295,182	368
2796	0.61	295,182	368

EIS: Solar Orbiter coordinated observations of long-term monitoring of a

2022-10-20T10:34:13 to 2022-10-20T11:06:14

Science Goal:

Program:

Target:

Pointing: xcen=-924 ycen=257,

saaIntervals hiIntervals

wavelength	cadence	FOVx,y	images
FeX		180,152	null
FeXVI		180,152	null
CaXVII		180,152	null
FeXXIV		180,152	null
FeXV		180,152	null
HeII		180,152	null
OV		180,152	null
FeXII		180,152	null
FeXXIII		180,152	null
FeXIV		180,152	null

IRIS: C1: South Pole

2022-10-16T01:06:40 to 2022-10-16T01:40:51

Science Goal: Very large coarse 64-step raster 126x175 64s Deep x 30

Program: C1: South Pole

Target: QS

Pointing: xcen=8 ycen=-950,

saaIntervals hiIntervals

wavelength	cadence	FOVx,y	images
1330	2.14	295,182	16
2832	2.14	295,182	16
1400	2.29	295,182	15
2796	2.14	295,182	16

IRIS: B1: AR tracking from limb to limb

2022-10-13T05:30:24 to 2022-10-13T05:48:30

Science Goal: Large coarse 64-step raster 126x120 64s Deep x 15 SJI cadence 3x faster Lossless compression

Program: B1: AR tracking from limb to limb

Target: AR

Pointing: xcen=794 ycen=435,

saaIntervals hiIntervals

wavelength	cadence	FOVx,y	images
1330	1.13	247,129	16
2832	1.13	247,129	16
1400	1.13	247,129	16
2796	1.13	247,129	16

IRIS: A1: QS monitoring

2022-10-07T04:33:04 to 2022-10-07T04:51:08

Science Goal: Large coarse 64-step raster 126x120 64s C II Si IV Mg II h/k Mg II w s Deep x 15 SJI cadence 0.5x faster

Program: A1: QS monitoring

Target: QS

Pointing: xcen=0 ycen=1,

saaIntervals hiIntervals

wavelength	cadence	FOVx,y	images
1330	1.13	247,129	16
2832	4.52	247,129	4
1400	1.13	247,129	16
2796	1.13	247,129	16

EIS: HOP130 04B/15

2022-10-06T19:47:47 to 2022-10-06T19:53:13

Science Goal: full_sun_slot_scan_2

Program:

Target:

Pointing: xcen=-473 ycen=-784,

saaIntervals hiIntervals

wavelength	cadence	FOVx,y	images
FeXIII		479,512	null
FeXVI		479,512	null
SiX		479,512	null
SX		479,512	null
SiVII		479,512	null
FeXI		479,512	null
FeXV		479,512	null
HeII		479,512	null
CaXVI		479,512	null
FeXII		479,512	null
FeVIII		479,512	null
FeXIV		479,512	null

IRIS: F1: Mid latitude scan (HOP 336) North #4

2022-08-28T23:39:32 to 2022-08-28T23:54:11

Science Goal: Large sparse 96-step raster 95x120 96s Deep x 8 Spatial x 2, Spectral x 2

Program: F1: Mid latitude scan (HOP 336) North #4

Target: QS

Pointing: xcen=128 ycen=449,

saaIntervals hiIntervals

wavelength	cadence	FOVx,y	images
1330	0.61	218,129	24
2832	0.61	218,129	24
1400	0.61	218,129	24
2796	0.61	218,129	24

IRIS: BBSO coordination, AR 13086

2022-08-25T20:00:17 to 2022-08-25T21:57:44

Science Goal: Large coarse 8-step raster 14x120 8s C II Si IV Mg II h/k Mg II w s Deep x 4 Spatial x 2, Spectral x 2 FUV spectrally rebinned x 4 SJI cadence 0.5x faster

Program: BBSO coordination, AR 13086

Target: AR

Pointing: xcen=-282 ycen=-469,

saaIntervals hiIntervals

wavelength	cadence	FOVx,y	images
1330	0.34	137,129	348
2832	2.03	137,129	58
1400	0.34	137,129	348
2796	0.34	137,129	348

IRIS: Flare studies, hot plasma

2022-08-24T08:44:36 to 2022-08-24T13:54:07

Science Goal: Medium sit-and-stare 0.3x60 1s C II Si IV Mg II h/k Deep x 8 FUV spectrally rebinned x 2

Program: Flare studies, hot plasma

Target: AR

Pointing: xcen=199 ycen=378,

saaIntervals hiIntervals

wavelength	cadence	FOVx,y	images
1330	0.47	61,67	660
1400	0.47	61,67	660
2796	0.47	61,67	660

IRIS: High-cadence flare program, AR 13078

2022-08-19T22:29:22 to 2022-08-20T00:12:38

Science Goal: High-Cadence Flare Program: .3 sec, flare linelist, Mg II h/k slow

Program: High-cadence flare program, AR 13078

Target: AR

Pointing: xcen=714 ycen=-437,

saaIntervals hiIntervals

wavelength	cadence	FOVx,y	images
2796	0.16	61,68	630

IRIS: HOP 336 South #2

2022-08-14T23:34:24 to 2022-08-15T00:24:17

Science Goal: Large dense 320-step raster 105.3x120 320s Deep x 8 FUV spectrally rebinned x 2

Program: HOP 336 South #2

Target: QS

Pointing: xcen=3 ycen=-685,

saaIntervals hiIntervals

wavelength	cadence	FOVx,y	images
1330	0.62	233,129	80
2832	0.62	233,129	80
1400	0.62	233,129	80
2796	0.62	233,129	80

247296 matches
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